Solar eclipse of April 11, 2051

Solar eclipse of April 11, 2051
Solar eclipse of April 11, 2051
	Map
Type of eclipse
Nature	Partial
Gamma	1.0169
Magnitude	0.9849
Maximum eclipse
Coordinates	71°36′N 32°12′E / 71.6°N 32.2°E
Times (UTC)
Greatest eclipse	2:10:39
References
Saros	120 (63 of 71)
Catalog # (SE5000)	9621

A partial solar eclipse will occur at the Moon's descending node of orbit on Tuesday, April 11, 2051, with a magnitude of 0.9849. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

The umbral shadow of the Moon will pass just above the north pole of the Earth. It will be the largest partial solar eclipse in 21st century.^[1]

The maximal phase of the partial eclipse (0.98) will be recorded in Barents Sea. The eclipse will be observed on the north-east of Europe and practically throughout in Asia, on north on Canada and Greenland and everywhere in US state Alaska.

Related eclipses[edit]

Solar eclipses of 2051–2054[edit]

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.^[2]

Solar eclipse series sets from 2051 to 2054
Descending node		Ascending node
Saros	Map	Saros	Map
120	April 11, 2051 Partial	125	October 4, 2051 Partial
130	March 30, 2052 Total	135	September 22, 2052 Annular
140	March 20, 2053 Annular	145	September 12, 2053 Total
150	March 9, 2054 Partial	155	September 2, 2054 Partial

Saros 120[edit]

This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon’s descending node of orbit.^[3]

Series members 50–71 occur between 1801 and 2195:
50	51	52
November 19, 1816	November 30, 1834	December 11, 1852
53	54	55
December 22, 1870	January 1, 1889	January 14, 1907
56	57	58
January 24, 1925	February 4, 1943	February 15, 1961
59	60	61
February 26, 1979	March 9, 1997	March 20, 2015
62	63	64
March 30, 2033	April 11, 2051	April 21, 2069
65	66	67
May 2, 2087	May 14, 2105	May 25, 2123
68	69	70
June 4, 2141	June 16, 2159	June 26, 2177
71
July 7, 2195